Technologies for Deviation of Asteroids and Cleaning of Earth Orbit by Space Debris

The present chapter presents the advanced design and technology of special equipment (SECSL) which uses concentrated solar light for deviation of asteroids and cleaning the space of debris. The elliptical orbit of any cosmic body as presented in Einstein ’ s general theory of relativity is rotating around the ellipse center. The trajectory of a cosmic body is permanently affected by the gravity of other moving cosmic bodies. In the case of asteroids (relatively small masses), orbit changes can lead to a collision with the Earth. At this very moment, our civilization has no efficient and reliable mean to destroy or divert a cosmic body heading toward the Earth. This new idea represents a “ light canon ” which uses concentrated solar light for deviation or vaporization of dangerous asteroids. The equipment is composed out of two parabolic mirrors (one large and one small) with the same focal point and coincident axes. The mirrors reflect the sunlight between them hence the term “ concentrated solar light. ” Next, a similar idea to the SECSL equipment is presented but applied to space debris caused mostly by humans and a new way of disintegrating satellites, spent rocket boosters, thrust chambers, etc. in the Earth ’ s atmosphere during reentry.


Introduction
Today, there is no reliable nor efficient system which can destroy or deflect asteroids or comets on a collision trajectory with the Earth. At this very moment, we cannot comprehend what could happen if an asteroid impacts the Earth. On April 13, 2029, we might experience just that because asteroid Apophis will pass below the orbit of low earth orbit (LEO) satellites and its exact trajectory cannot be predicted.
Albert Einstein, in his general theory of relativity, says that the elliptical orbit of any cosmic body is rotating around the ellipse center (i.e., the perihelion of the orbit is moving continuously). The elliptical orbit or trajectory of any cosmic body (i.e., asteroids, comets, etc.) can be permanently altered by the gravity of other asteroids and planets. Due to this reason, asteroids can be involved in collisions that cause sudden trajectory changes. The trajectory change could one day be toward the Earth, because asteroids have relatively small masses; thus a change in its trajectory is significant.
According to estimates, there are over 150 million asteroids in our solar system, most of them are grouped in what is called an asteroid belt (see Figure 1) and have trajectories passing close to the Earth (see Figure 2). NASA's revised estimate of the number of near-Earth asteroids provided by Wide-field Infrared Survey Explorer (WISE) during the NEOWISE project had the number of larger than 100-m objects which are considered medium-to large-sized asteroids at 500. Near-Earth asteroids smaller than 100 m were not studied, and at a later time, near-Earth comets will be analyzed.  For asteroids larger than 1000 m, the revised number is down to 981 from a prior estimate of about 1000. Out of the 981 large-sized asteroids, NASA managed to estimate with great precision the size of each individual.
The number of asteroids that disintegrate into the atmosphere is surprisingly very high (see Figure 3) which demonstrates that the problem with asteroid impact is very alarming.
Two proposed solutions for the Earth's protection against asteroids are synthesized in [1]. The first protection method is presented in Figure 4, and it relies on capturing small celestial objects. The second method is presented in Figure 5, and it relies on a satellite carrying a nuclear-powered laser which deflects asteroids through local vaporization (laser ablation).
Other solutions propose asteroid gravity tractor, kinetic impact, nuclear explosive devices, etc. It is quite clear that these solutions are not completely satisfactory.  Asteroids can be very large objects, most of them are rotating conglomerates formed through accumulation of debris after colliding with other asteroids.
Measurements of rotation rates of large asteroids located in the asteroids belt yielded no upper limit. No asteroid with a diameter larger than 100 m has a rotation period smaller than 2.2 h. However, a solid object formed through accumulation of debris after collisions between asteroids should be able to rotate much faster. Due to these issues, the Earth's protection against asteroids has no satisfactory solution just yet.
Also in the near-Earth region, there are not only asteroids and comets, there's also man-made debris as a result of space exploration missions manned and unmanned. Man-made space debris already represents a great threat to the safety of space exploration and exploitation. Most of the space debris is concentrated in the near-Earth space region in the low earth orbit (LEO) and geostationary earth orbit (GEO) (see Figures 6 and 7). Space debris are composed of nonfunctional rocket boosters, spent rocket upper stages, paint flakes, chunks of slag from solid rocket motors, old science experiment equipment, nonfunctional satellites, various fragments which are the result of collisions, satellite components destroyed by missiles, and materials detached from the International Space Station (ISS) [4].
Just like asteroids, space debris can be classified by their dimensions: • Category I: size <1 cm-can cause significant damage to vulnerable parts of the satellite.
• Category II: size 1 to 10 cm-can cause serious damage to or destroy a satellite; there is no effective shielding against this category of debris.
• Category III: size >10 cm-can destroy a satellite by collision; it can be tracked, and the satellite can perform evasive maneuvers to avoid collision.  Today, the growth of space activities is exponential, but this growth has generated an important problem: the need for rapid disintegration of space debris after reentry in the Earth's atmosphere. Space debris as stated earlier represents nonfunctional man-made objects or fragments of such objects. Only 6% of catalogued objects are functional, the rest of them are space debris [3]. At the end of their operational life, satellites reenter the Earth's atmosphere being disintegrated through burning initiated by the friction with air. This is happening for the final rocket stages which become space debris after the propellant has been depleted. In many cases the space debris fallen on the ground had large dimensions (helium tanks, thrust chambers, propellant tank, pressure sphere) [5].
The lifetime of a man-made object is very long; for example, satellites of the Satellite Pour l'Observation de la Terre or Satellite for Observation of Earth (SPOT) family placed on a Sun-synchronous orbit can orbit for about 200 years at 822 km altitude representing a high risk for other satellites [6]. Regulations were issued for direct deorbiting of satellites after finishing their operational life, but these regulations do not solve the need for rapid burning of satellites in the atmosphere; thus big chunks of unburned metal could fall on the ground [7].
The European Space Agency (ESA) came with a proposal to solve this problem under the name of "Design for Demise," according to which space equipment design must take into account the on-ground safety requirements [8].
The "Design for Demise" proposes that separation of satellite into components due to the centrifugal forces should be done during the reentry procedure. Although this is a good idea, it still does not respond to the need of rapid burning in the atmosphere, and again big chunks of unburned metal could fall on the ground.
For each of the upper-mentioned problems, there is a potential solution in the form of a system or a new way of designing space equipment. In the next chapter, each system will be presented in detail.
2. Special equipment which uses concentrated solar light for earth protection against asteroids: "light gun" The special equipment which uses concentrated solar light for Earth protection against asteroids proposed in this paper could be placed on a solar orbit close to the Earth or on the Earth's orbit. This special equipment represents a system which includes one large and one small parabolic mirrors both highly reflective and with the same focal point. The reflectivity of a mirror is given by reflective foils (or plates) which are stretched on a lightweight parabolic support for the mirror. The light rays coming from the Sun are focalized by the large parabolic mirror onto the focal point; afterward they are reflected by the small parabolic mirror as a group of parallel rays which pass through a central hole located in the center of the large parabolic mirror. A mirror tube attached to the large parabolic mirror by means of an articulation permits the orientation of the concentrated light beam as required (see Figure 8).
The role and functions of the main components: 1. Large parabolic mirror. Role: capture and focus sunlight onto the common focal point.  The SECSL is table in space; according to the law of momentum conservation, the sum of all light impulses is zero. However, when the light beam is directed toward the target, this balance is changed, and compensation forces must be applied to keep the system in position (i.e., with the concave side of the large parabolic mirror oriented toward the Sun).

Estimating the power of a SECSL system
Solar power is the key future for our civilization to expand in space. The main component of this power is electromagnetic radiation. The spectrum of solar radiation is the spectrum of a black body having a temperature of 5800 K [9]. The electromagnetic radiation is emitted in a broadband of frequencies. Electromagnetic energy is initially emitted in the range of gamma rays, as a result of nuclear fusion reactions. Gamma rays during their travel from the Sun's core to the surface are converted into low-energy photons. Thus the Sun does not emit gamma rays; it emits only X-rays, ultraviolet light, visible light, infrared light, and radio waves. The spectrum of nearly all solar electromagnetic radiation striking the Earth's atmosphere ranges from 100 nm to 1 mm.
In Figure 9 the power emitted by the Sun under the form of X rays and ultraviolet is low. Most of the power is emitted in the range of visible light. Infrared and radio frequencies have less power. Assuming the SECSL is placed near the Earth, the irradiance can be assumed to be E e = 1360 W/m 2 .
Both mirrors are made from gold-plated Mylar foil with remarkable reflectivity coefficient [10]. Figure 10 shows that for most frequencies, gold has a reflection coefficient of R g = 0.98 compared to aluminium or silver. In the case of the SECSL, the best foil should be made of gold-plated fine and thin graphite fabric due to gold's remarkable reflection coefficient and graphite's high heat transfer coefficient and high emissivity coefficient.
If the large parabolic mirror is oriented with the reflective (concave) face towards the Sun, the amount of energy captured is maximized.
For example, if the large mirror has a radius of r = 10 m and assuming the solar irradiance is E e = 1360 W/m 2 , the total collected power is The total collected power is significant. However, when this radius increases, the power collected from the Sun becomes very high. Table 1 shows the correlation between the SECSL mirror diameter and the amount of collected power. As shown in the table, when the radius of the large parabolic mirror r = 50 m, the collected power is P = 10681.4 kW. Such a mirror is relatively easy to be built in space due to the absence of gravitational forces.
For a simple sample calculation, assume that a SECSL having a radius of large parabolic mirror, r = 50 m, is focused on an iron asteroid for 10 s. Consider iron properties listed in the literature [11]:   The heat quantity needed in order to vaporize 1 kg of iron can be calculated: Reading from Table 1 the power for the mirror with a radius r = 50 m, in 10 s the power beam into the asteroid is This total energy can vaporize a mass of iron given by Hitting the asteroid continuously (hundreds or thousands of times) in this manner, it can be deflected from a collision trajectory with the Earth. Even the trajectory of massive asteroids can be changed. Due to local vaporization of the asteroids, mass leads to the apparition of a reaction force produced by the expanding vapors.
In space the construction of such a gigantic system should be easier due to the absence of gravity. Calculations done using the above equations show that an SECSL having the radius of the large parabolic mirror r = 10 km can send a beam of concentrated light into the asteroid at a power of 0.427 terawatt. Such a power can vaporize an iron asteroid having the mass of 100 tons in just 8 s.
The time required to destroy or deflect an asteroid using the SECSL system is reasonably low. Practically, the asteroid can be destroyed in a few minutes because obviously the SECSL beam hits the target with the speed of light.

Heat transfer calculations
Simple calculations show that SECSL works properly both near the Earth (where irradiance Ee = 1360 W/m 2 ) and at 0.1 AU distance from the Sun (where irradiance is Es = 136,000 W/m 2 ).
Assume that a SECSL placed near the Earth having the large parabolic mirror radius r LPM = 10 km and the radius of the small parabolic mirror r SPM = 1.25 km; this system is capable of concentrating the sunlight by a factor of 64.
Consider that the reflection coefficient for a gold-plated foil R gf/p = 0.98 and the emissivity of carbon fabric/plate e c ≈ 1.
Assume that the whole power absorbed by the gold-plated foil is radiated according to Stefan-Boltzmann law: In Eq. (1) σ = 5.67Á10 À8 W/m 2 K 4 represents the Stefan-Boltzmann coefficient for black body radiation. Using the given data, thermal balance is achieved at T = 410 K (t = 137°C), which is under the maximum allowable working temperature for carbon composites with polymeric matrix (t = 280-300°C).
Considering that the thickness of the gold-plated foil is δ = 0.05 mm and the average thermal transfer coefficient for graphite is λ = 80 W/m K at t = 137°C, the temperature difference Δt needed for heat transfer from the gold reflective face to the rear carbon face is given by the following thermal balance equation: For the given equation, the thermal difference necessary for heat transfer would be Δt = 0.001°C; the result shows that heat is quickly transferred from the goldplated face to the graphite fabric/plate due to the high thermal conductivity of the graphite and small thickness.
At the beginning of this chapter, we've stated that SECSL works properly even at 0.1 AU from the Sun, where the irradiance is 100 times stronger. Considering the same constants and mirror dimensions as before and using Eq. (1) we find that the surface temperature of the small parabolic mirror is T SPM = 1296 K (t SPM =1023°C) which is under the melting point of pure gold (1064°C). Thermal balance at the surface of the large parabolic mirror is achieved at T LPM = 476 K (t LPM = 203°C) still under 280-300°C-the working temperature limit for carbon fiber composite with polymeric matrix.

SECSL mass calculation
In Figure 11 the cell design is based on triangular shapes. It can be either hexagonal or rectangular cells, i.e., if rectangular cells are used, it yields a light structure, but the stability is reduced compared to the design of triangular cells. When using gold-plated foils, the structure bars can be square and straight. If goldplated plates are used, the bars must be curved according to the parabolic surfaces of the mirrors which in this case results in a higher accuracy in focusing the light.
Such a construction can be relatively easily built in space if "SpiderFab" robots are used (see Figure 12) [12]. Preliminary calculations show that the resistance structure of the large parabolic mirror can be built from 528 bars with 9.3 m in length. If the bars are square tubes made from titanium having dimensions of 20 Â 20 Â 0.2 mm 3 , calculations show that the total mass is 357 kg. If graphite fiber composites are used instead of titanium, the mass of the large parabolic mirror decreases to about one-third due to the extremely low density of these materials.

Solar-thermal system for deorbiting space debris
This system is similar to the one presented in Chapter 2, composed of two parabolic mirrors, a large one and a small one (see Figure 13). Just like in the case of SECSL, the mirrors are made from very thin composite material (graphite fiber) plated with gold foils or gold plates on the concave face. The concave faces of the two mirrors face each other having the same focal point. The solar light rays which are parallel to the axis of the large parabolic mirror are reflected into its focal point and onto the small parabolic mirror and form parallel rays which are directed along the common axis. The diameter of the concentrated light beam is the same as the diameter of the small mirror ("d"). The concentrated light beam passes through a cutout (hole) in the center of the large parabolic mirror with diameter d + . The hole in the large parabolic mirror is closed by a gold-plated shutter.
The system operates as follows: the system is oriented with the large parabolic mirror to the Sun using the attitude thrusters, while the shutter is closed. The light guide tube is aligned with the space debris, and the faces of the lens are curved at the appropriate radii in order to focus the light on the space debris. When the shutter opens, the light coming from the Sun is focused by the large parabolic mirror in the common focal point and then is reflected by the small parabolic mirror toward the hole "d + " and the light guide tube. At the end of the light tube, the light is focused by the lens in a focal point which is positioned onto the space debris. The focused light locally vaporizes/ionizes the space debris material. The thrust force created pushes the space debris toward the Earth surface where it burns in the atmosphere.
When the shutter is closed, the light rays are sent back toward the small parabolic mirror and back to the Sun.
An alternative to the parabolic mirror system is the Cassegrain-type or Gregorian-type solar-thermal system. These systems are used in manufacturing optical telescopes or radio antennas [13].
Basically, a Cassegrain reflector (see Figure 14) [14] is a combination of a large concave and a small convex (hyperbolic) mirror. This design permits placing a focal point at a convenient location behind the large parabolic mirror using a compact mechanical system.
On the other hand, the Gregorian reflector [15] uses a small concave (parabolic) mirror with a focal point that doesn't coincide with the focal point of the large parabolic mirror (see Figure 14).
Although the Cassegrain-type and the Gregorian-type solar-thermal system can focus the light in a single point placed behind the large parabolic mirror, it is more difficult to change the focal point distance and direct the concentrated light beam onto the space debris.

Orbits for the solar-thermal system for space debris deorbiting
This system can be placed on a geocentric orbit, heliocentric orbit, or Sunsynchronous orbit. The most advantageous is the Sun-synchronous orbit (helio-

Lens design
The lens that is placed in the light tube has the role to focus the light on a very small area in order to assure very high power density. Theoretically, the energy can be focused on a geometric point. In reality due to chromatic aberration and shape errors, light is not focused quite precisely. The lens presented in Figure 15 is made out of and elastic material filled with a colourless liquid.
Approximating surfaces "S1" and "S2" with spheres having radii "r 1 " and "r 2 ," respectively, assuming the thickness of the lends is denoted as "d" and neglecting the optical effect of transparent elastic material (which is very thin) if the refractive index of the liquid is "n," the focal distance "f" of the lens is given by the following equation [13]:  In order to simplify the case of such model, consider r 1 = r 2 = r: Eq. (8) shows that for a given n and d, when r ─ › ∞ (i.e., low pressure of liquid inside the lens), f ─› ∞, i.e., theoretically the system can hit the target (space debris) at any distance. However, due to aberration and imprecision of lens dimensions, this distance is limited. Lens operation is illustrated in Figure 16.
The temperature of liquid must be kept in an appropriate range for preserving the liquid state (avoiding of freezing). A resistor fed by battery charged by solar cells heats the liquid which is circulated permanently by a pump with a low speed. The electro-valve is normally opened. When hitting the space debris is necessary, the electro-valve is closed, and the liquid bends the lens to the necessary curvature. Some suitable liquids and reflective indexes are given in Table 2 [17].
The transparent elastic material can be polydimethylsiloxane (PDMS) which has good optical properties and large elongation and is highly transparent (over 96%) in the range of visible wavelengths. PDMS refractive index is n PDMS = 1.41. In a terrestrial application, such an elastomeric membrane having 60 microns in thickness was used in manufacturing convex lenses [18]. The refractive liquid used in that design was water.  3.3 Estimated power, specific impulse, and thrust calculations

Estimated power calculations
The space debris is made of various metals (aluminium, titanium, carbon fiber composite, steel, etc.). For example, consider a space debris made out of aluminium. In Chapter 2 we've considered the space debris made out of iron.
Consider aluminium properties listed in the literature [19]. For simplicity they are considered constant for a wide range of temperatures: Making the appropriate substitutions in Eq. (9) results E vap ¼ 0:9 Á 2743 þ 398 þ 1:18 Á 2743 À 933:3 ð Þ þ 10518 ¼ 15520 kJ=kg (10) The total energy needed to ionize aluminium atoms after vaporization is In Table 3 the amount of aluminium that the system can vaporize and ionize in 1 s is presented.

Estimated specific impulse and thrust calculations
The process of generating reaction force due to material ablation is very complex. This effect was observed by pointing a laser to a material surface [20]. In this present case, the process should be similar.
In the case of laser rays, ablation takes place when the material is removed from a substrate through direct absorption of laser ray energy. As a first condition, the radiation energy must exceed a given threshold, which is less than 10 J/cm 2 for metals, 2 J/cm 2 for insulating inorganic materials, and 1 J/cm 2 for organic insulation materials [20].
The solar-thermal system discussed here (see Table 2, case no. 1) satisfies this requirement because, even when the power of the smallest mirror is 0.98 Â 0.98 Â 88.4 = 84.9 kW, it provides an energy of 10 J in 1.18 Â 10 À4 s [20].
Another condition is related to the energy absorption mechanism. Chemical composition, microstructure, and morphology of material strongly influence the absorption of heat.
Heating debris must be sufficiently fast for homogenous nucleation and expansion of vapor bubbles and ions.
Some simulations done for interaction of laser rays have shown that [21]: • The degree of light absorption increases as the cavity deepens.
• Maximum energy absorbed by the cavity is around 80% of the total energy of radiation.
• The radiation is multiple times reflected by the cavity, and as a result, the energy is highly concentrated at the center and the bottom of the cavity and forms the final conical shape of the cavity.
• The surface temperature is much higher than the normal boiling point.
• In order to be able to remove the material, it must have a homogenous boiling regime and evaporation; the power intensity must be over 108 W/cm 2 .
Note: The mentioned simulations have been conducted only for iron, not for aluminium or other materials currently used in manufacturing satellites and space equipment, but the effect should be similar ( Figure 17).
In some experiments a specific impulse of around 4000 s was measured for carbon and aluminium in ionized state produced by the laser ray [23]: During those experiments the following observations were made: • The speed of the ejected atoms and implicitly Isp is inversely proportional to the square roots of the atomic mass of ablated material; the lighter the element the higher the specific impulse.
• Thrust tends to increase with atomic mass of ablated material.
• The speed of the ejected atoms was independent of angle at 22 cm away from the target.  Table 3.
The quantity of aluminium vaporized by the system in 1 s.
For the case where Isp has a known value, one can evaluate the thrust force by the following equation: where g 0 represents the gravitational acceleration at the Earth's surface (g 0 = 9.81 m/s 2 ). _ m represents the mass of ions ejected in 1 s. Momentum coupling coefficient C m is another method for thrust evaluation [20]. This coefficient characterizes thrust production efficiency. The coefficient is determined as the thrust to laser power ratio. This parameter determines the minimum light power required to produce a 1 N thrust: According to the above reference, C m max Al = 6Á10À5 N/W for aluminium. That means that in the case of ablation of a space debris made of aluminium using a solarthermal system with a power of P = 88.4 kW, the thrust force resulted is In case the large parabolic mirror has a diameter of r lpm = 25 m, the thrust force is In both cases the thrust force is remarkably high and can deorbit space debris with just a few hits.

A new design of space equipment for rapid disintegration in atmosphere after reentry
This new design is inspired by the tragic loss of the Space Shuttle Columbia's crew on February 1, 2003 [24]. Columbia disintegrated over Texas and Louisiana when it reentered the Earth's atmosphere. During the launch of the space shuttle, a piece of foam insulation struck the left wing of the orbiter deteriorating its ablative protection [24]. When time came for the space shuttle to reenter the Earth's atmosphere, the damage caused by the foam insulation allowed hot air to penetrate into Figure 17. The effect of a focused light ray on a material [22]. the wing creating an irregular hole. Air entered the left wing with high speed, quickly became very hot when stagnating, and destroyed the internal structure of the wing.

Lessons learned after the Space Shuttle Columbia disaster
During the reentry phase, shock waves produced by hypersonic velocities and the frictional effect of the atmosphere began to heat Columbia's surface. The temperature varied depending on location: the orbiter's nose and leading edges of the wing experiencing temperatures greater than 1538°C [25].
The breach created during launch in the ablative protection of the left wing allowed for hot gases to penetrate the wing and to advance in the same direction inside the wing and to the fuselage (see Figure 18). This phase became known as "phase I" from "Initialization." During the "Initialization" phase, the wing lost its aerodynamic characteristics, and the destruction process was extremely short, lasting from 13:59:37.5 GMT to 13:59:39.7 GMT (2.2 s) (see Figure 19) [25].
The "Acceleration" phase quickly followed the "phase I" which lasted for 0.07 s. The destruction continued with total dispersal of the space vehicle and burning in the atmosphere (see Figure 20). This phase can be called "phase D" from "Dispersal" and lasted for 55 s ( Figure 21).

Space equipment for rapid disintegration during atmosphere reentry
As presented in Chapter 1, ESA's "Design for Demise" concept must be implemented in every space equipment. Following those guidelines, the present paper presents a new vision of that concept. It is known that satellite equipment is covered by a protection box which shields them against environmental factors such as cosmic radiation, solar wind, light (ultraviolet, visible, infrared), cosmic dust, and rarefied atmosphere. Usually, this box is a prism which has a pretty low dynamic drag, and, as a result, reaching high temperatures on the surface of the satellite is delayed; therefore the satellite disintegration is delayed during reentry. The situation is even more critical in the Figure 19. Initiation phase of the destruction process (phase I) [25]. case of the last stages of launching rockets which have a good aerodynamic shape in order to have a low aerodynamic drag during the ascending phase of the launch.
According to the space equipment design presented in this paper, special doors must be incorporated in the external fairing of the space equipment. The holes in the fairing can have any shape (rectangular, triangular, hexagonal, circular, etc.) depending on the position of the fairing. Doors fitted on every hole must be articulated by a cylindrical articulation (i.e., to permit a rotation of the door around an axis); this allows the door to open to the interior of the box when external pressure increases and to close when the pressure inside the fairing is higher than the external pressure. The door is fixed to the fairing through brazing with low fusible metals or strong resins (Loctite, Araldite) which decompose at low temperatures (150-200 to 700°C in special cases). Both the resin and metallic alloys must be extremely resistant at low temperatures but must lose their strength when temperature reaches several hundreds of degree Celsius. In in the early stages of the reentry, the epoxy resins decompose at temperatures between 150 and 200°C, and the braze alloys are melting when the local temperature reaches 200-700°C. As a result, the doors (covers) are pushed inside the fairing, and the external air enters inside where stagnates reach extremely high temperatures. The new external geometry of the space equipment leads to an increase of aerodynamic drag and converts kinetic energy into heat, which enhances the burning process.
By placing more doors on the fairing, no matter how the space equipment rotates during reentry, at least one door is opened by the dynamic pressure, and the rest of them are closed by the same dynamic pressure. Heating inside the fairing is maximum due to air stagnation, which leads to a rapid disintegration of the space equipment.
If the covers (doors) are not articulated, they are pushed inside the equipment by the ambient pressure acting on the surface of the fairing. Being pushed inside, the doors allow the air to flow inside the fairing around the equipment, but does not stagnate; thus heating does not occur, and the aerodynamic drag is low. For this reason the heating hate will be lower than when articulated covers are used.
For an even faster disintegration of the space equipment, the satellite components are wrapped in 0.05-mm thick aluminium or magnesium foil. These lightweight foils will burn first followed shortly by the equipment. This new technology can be seen in Figures 22-27.
Applying this design will determine the space debris to be disintegrated according to Space Shuttle Columbia's tragic disintegration phases I, A, and D.